• Source: 5176 Yoichi

5176 Yoichi, provisional designation 1989 AU, is a background asteroid from the central regions of the asteroid belt, approximately 17 kilometers (11 miles) in diameter. It was discovered on 4 January 1989, by Japanese astronomers Seiji Ueda and Hiroshi Kaneda at the Kushiro Observatory on Hokkaido, Japan. The likely elongated asteroid has a brightness variation of 0.45 magnitude, and occulted a star in the constellation Cetus in November 2014. It was named for the Japanese town of Yoichi.




Orbit and classification


Yoichi is a non-family asteroid from the main belt's background population. It orbits the Sun in the central main-belt at a distance of 1.9–3.5 AU once every 4 years and 5 months (1,609 days; semi-major axis of 2.69 AU). Its orbit has an eccentricity of 0.31 and an inclination of 8° with respect to the ecliptic.
The body's observation arc begins with its first observations as 1935 YH at Johannesburg Observatory in December 1935, or 53 years prior to its official discovery observation at Kushiro.




Physical characteristics


Yoichi is an assumed S-type asteroid, while the body's albedo is rather indicative of a carbonaceous C-type asteroid (see below).




= Rotation period

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In November 2015, photometric data of Yoichi was taken by astronomers at the Oakley Southern Sky Observatory in Australia. However no rotational lightcurve could be constructed. The asteroid's brightness amplitude was 0.42 magnitude (U=n.a.), indicative for an elongated shape. As of 2018, the body's rotation period, pole and shape remain unknown.




= Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Yoichi measures between 15.68 and 19.49 kilometers in diameter and its surface has an albedo between 0.05 and 0.0849.
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0777 and a diameter of 16.54 kilometers based on an absolute magnitude of 12.3.




= Occultation

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On 2 November 2014, Yoichi occulted 8.4 magnitude star HIP 14421 in the constellation Cetus, causing a magnitude drop from 8.4 to 14.1 during 2.8 seconds. The occultation was visible over Southern Japan, Eastern China, as well as from Southern California to North Florida. The asteroid's 23-kilometer-wide shadow had a speed of approximately 6.8 km/s. An approximate diameter of 20 kilometers was assumed for the asteroid.




Naming


This minor planet was named after the Japanese town of Yoichi on Hokkaido, where the discovering Kushiro Observatory is located. The official naming citation was published by the Minor Planet Center on 4 August 2001 (M.P.C. 43189).




References






External links


Asteroid Lightcurve Database (LCDB), query form (info Archived 16 December 2017 at the Wayback Machine)
Dictionary of Minor Planet Names, Google books
Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
Discovery Circumstances: Numbered Minor Planets (5001)-(10000) – Minor Planet Center
5176 Yoichi at AstDyS-2, Asteroids—Dynamic Site
Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
5176 Yoichi at the JPL Small-Body Database

Kata Kunci Pencarian:

• 5176 Yoichi
• Yōichi
• Meanings of minor-planet names: 5001–6000
• Hiroshi Kaneda
• List of minor planets: 5001–6000
• Seiji Ueda
• List of named minor planets: 5000–5999
• List of named minor planets: Y
• 5175 Ables
• Omicron Virginis